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Spot evolution in the eclipsing binary CoRoT 105895502
DOI: 10.1051/0004-6361/201834516 Bibcode: 2019A&A...623A.107C

Schmitt, J. H. M. M.; Czesla, S.; Wichmann, R. +1 more

Stellar activity is ubiquitous in late-type stars. The special geometry of eclipsing binary systems is particularly advantageous to study the stellar surfaces and activity. We present a detailed study of the 145 d CoRoT light curve of the short-period (2.17 d) eclipsing binary CoRoT 105895502. By means of light-curve modeling with Nightfall, we de…

2019 Astronomy and Astrophysics
CoRoT Gaia 9
CSI 2264: Simultaneous optical and X-ray variability in the pre-main sequence stars of NGC 2264. II. Photometric variability, magnetic activity, and rotation in class III objects and stars with transition disks
DOI: 10.1051/0004-6361/201935466 Bibcode: 2019A&A...628A..74G

Micela, G.; Stauffer, J.; Sciortino, S. +6 more

Context. Pre-main sequence stars are variable sources. In diskless stars this variability is mainly due to the rotational modulation of dark photospheric spots and active regions, as in main sequence stars even if associated with a stronger magnetic activity.
Aims: We aim at analyzing the simultaneous optical and X-ray variability in these st…

2019 Astronomy and Astrophysics
CoRoT 6